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Previous literature has shown that the introduction of homogeneous perforation on plates and cylinders decreases aerodynamic drag. Here, it is shown that the opposite is true for a sphere; drag can increase with porosity. Hollow porous spheres exposed to a uniform free stream are studied experimentally using force and flow field measurements. The parameter space encompasses moderate to high Reynolds numbers ($5 \times 10^4 \leq \textit{Re} \leq 4 \times 10^5$) and porosities ranging from $0\,\%$ to $80\,\%$. The main conclusion is that drag increases with porosity, at super-critical Reynolds numbers, for all studied porosities. At low porosities (less than $9\,\%$), the effect of porosity on drag can be explained by shifts in the separation point. At higher porosities the drag increase cannot be explained by separation shifts, and instead is explained by two competing forms of kinetic energy dissipation: (i) shear on the macro-scale of the body, and (ii) hole losses from flow through the pores. The former generally decreases with porosity, as bleeding flow passing through the body decreases the characteristic velocity difference in the body-scale wake. In a sphere, hole losses increase with porosity sufficiently fast to overcome decreasing body-scale shear losses, in contrast to plates and cylinders where this is not the case. Relatively weak wake vortex structures, and associated low drag coefficient at zero porosity, for a sphere reduce the impact of wake bleeding. Moreover, fluid entering the fore of a sphere can exit perpendicular to the free stream, further reducing wake bleeding while still contributing to hole losses.
This work aims to complement the description of the atomisation process in a typical commercial pressure-swirl atomiser. Conventional characterisation focuses on the final spray, where established experimental techniques allow for measuring spherical droplets in a dilute regime. However, the early stages of atomisation involve distorted liquid structures with complex interface morphology that challenge both experimental and numerical approaches. While numerical simulations with interface-capturing methods have provided access to this region, they currently remain computationally prohibitive to follow the atomisation process until the formation of the final spherical droplets. To characterise the evolving interface morphology, we propose analysing the curvature distribution obtained from both simulations and two-photon laser-induced fluorescence (2P-LIF) imaging. This curvature-based methodology, recently developed to characterise numerical sprays (Palanti et al. Intl J. Multiphase Flow 147, 2022, 103879; Ferrando et al. Atomiz. Sprays 33, 2023, 1–28), is here extended to experimental data. Both approaches are compared with available phase Doppler anemometry (PDA) measurements performed further downstream on spherical droplets. The morphological evolution of the atomising spray is interpreted through curvature statistics, which provide a unified framework applicable to all atomisation stages. When applied to spherical droplets, the curvature distribution recovers the conventional drop size distribution, linking early interface deformation to the final spray structure. The birth of this final drop size distribution can thus be observed by comparing the three approaches – numerical simulation limited to the early stage of atomisation, curvature derived from 2P-LIF images limited to two-dimensional (2-D) contour analysis, and PDA measurements of the dilute spray. The results show that curvature properties evolve in a way that can be directly representative of the final spray even at early atomisation stages.
A lattice Boltzmann method is adopted to investigate the breakup of surfactant-free and surfactant-laden droplets in both regular and irregular T-junction microchannels. During droplet neck contraction, the neck thinning shifts from inertia dominated to interfacial tension dominated, causing spontaneous rapid neck collapse due to Rayleigh–Plateau instability. For the regular rectangular microchannels, we find that the prerequisite for the spontaneous breakup of a surfactant-free droplet is that the local capillary pressure in the triggering area exceeds the Laplace pressure difference between the inside and outside of the droplet neck. Results show that the critical neck thickness $\delta _\textit{cr}^{*}$ for the droplet spontaneous breakup increases with increasing height-to-width ratio $\chi$ of the microchannel in both surfactant-free and surfactant-laden systems. The presence of surfactants decreases $\delta _\textit{cr}^{*}$ at the identified $\chi$, while the surfactant effects are gradually enhanced as $\chi$ increases. Subsequently, a constriction section is incorporated into the upper microchannel wall to establish an irregular microchannel. As constriction depth (length) increases, $\delta _\textit{cr}^{*}$ linearly decreases (increases) in the surfactant-free system, while $\delta _\textit{cr}^{*}$ exponentially decreases (linearly increases) in the surfactant-laden system. Four empirical formulas are proposed to predict the values of $\delta _\textit{cr}^{*}$ under varying constriction depths and lengths in the two systems.
The chronology of Late Pleistocene and Holocene aeolian sand activity in midcontinent North America provides important insight into paleoenvironmental change and associated surface processes. Near the limit of Marine Isotope Stage 2 glaciation of the Huron-Erie Lobe (Laurentide Ice Sheet) in south-central Indiana, aeolian sand deposits found along the eastern margin of outwash plains in the East Fork and West Fork White River valleys provide an opportunity to test the causal mechanisms for aeolian sand activity. Twenty-five optically stimulated luminescence ages on aeolian sand and four radiocarbon ages on gastropod shells document two phases of aeolian sand activity. The first phase, between 26 and 19 ka, records deflation from active outwash plains in the East Fork and West Fork White River valleys during and after the local glacial maximum. These ages overlap with the chronology of Huron-Erie Lobe advance into and out of the White River drainage basin based on a radiocarbon-dated slackwater succession. The second phase, between 16 and 12 ka, records reworking of older aeolian sand and outwash during a period of no-analog vegetation during the Bølling-Allerød/Younger Dryas and is in general agreement with the timing of dune activity from previous studies in the Great Lakes region.
A large-scale outcrop was exposed along the newly constructed road access to the Kumamoto Earthquake Museum “KIOKU” (former Tokai University Aso Campus). Multiple layers of tephra and paleosols cover the Sawatsuno lava (27 ± 6 K-Ar ka) in this outcrop. Three (3) characteristic tephra layers: Kusasenrigahama Pumice (Kpfa: ca. 32.5 cal ka BP) from Kusasenrigahama crater in Aso caldera, Aira Tn (AT: ca. 30 cal ka BP) and Kikai Akahoya (K-Ah: ca. 7.3 cal ka BP) from southern Kyushu are intercalated between thick sandy volcanic ash layers erupted from the post-caldera volcanoes of Aso caldera. Thirteen (13) radiocarbon ages were obtained from soil samples and charcoal fragments. Among these, a sample just below AT shows a younger age, indicating that the upper soil/tephra sequence including AT, was re-deposited on ground surface at the time immediately after ca. 13.4 cal ka BP indicated by this age. This suggests that the duplicated sequence, confirmed by our detailed dating is a product of either near-surface hidden faulting or a small local landslide associated with one of the paleoseismic events similar to the 2016 Kumamoto Earthquake.
This article attempts a first historical periodisation of the checkered history of the French Southern Islands in the Indian Ocean. Beginning with early extractive activities during the 18th and 19th centuries and followed by colonial ambitions during the first half of the 20th century, the article also discusses the more recent efforts of the French government to reinforce sovereignty in the form of permanent bases, especially during the 1950s and 1960s. The most recent period covered of scientific affirmation and ecological restoration (1970s–2006) introduces a solid historical perspective on the still ongoing efforts (from 2006 onwards) of reinforced patrimonialisation and environmental protection of the French Southern Islands. Throughout all periods, our main attention is directed towards various forms of projects. Indeed, the project perspective allows to uncover largely forgotten ambitions and shows that the history of the French Southern Islands is closely connected to larger historical developments in the entire Antarctic and sub-Antarctic region.
Loess–paleosol sequences (LPSs) provide valuable archives of Quaternary paleoenvironments. Here we present new data from the Baix LPS, comprising the entire Late Pleistocene. The Baix LPS is located at the western edge of the Rhône Rift Valley, France, in the transition zone from the presently temperate to the Mediterranean region of Europe. This LPS provides a missing link between the analyzed LPSs in the presently temperate regions farther north and those in the Mediterranean region. Reddish Btg horizons of a Stagnic Luvisol at the base of the Baix LPS represent the remains of an MIS 5 pedocomplex formed under warm and, at least temporarily, relatively moist conditions. Two brown Bw horizons of truncated Cambisols have been preserved in the overlying MIS 5a/4 to MIS 3 deposits. The upper Bw horizon is associated with large carbonate nodules, indicating that considerable amounts of calcium carbonate were leached from a former MIS 3 Cambisol and accumulated in the underlying loess unit. This truncated MIS 3 Cambisol is very similar to the MIS 3 paleosol remains in the LPS Collias that we investigated 87 km farther south in the present Mediterranean climate. No paleosols were observed in the late MIS 2 deposits.
Land degradation in China’s dryland regions presents a significant challenge to ecological sustainability and socio-economic development. Despite existing frameworks such as the Land Administration Law and the Regulation on Land Reclamation, implementation is impeded by fragmented legal provisions, unclear responsibilities, weak enforcement and limited public participation. Addressing these issues requires comprehensive legal reforms, capitalizing on the opportunity provided by the drafting of the Ecological Environment Code. Key reforms include introducing criminal sanctions for non-compliance, clarifying stakeholder responsibilities and enhancing inter-agency coordination. Promoting increased involvement from both the public and private sectors is essential. Strengthening the legal framework will improve reclamation outcomes, support sustainable land management and facilitate ecological restoration, offering valuable lessons for global land reclamation efforts facing similar degradation challenges.
Stéphane Dees, Banque de France and Bordeaux School of Economics, University of Bordeaux, France,Selin Ozyurt-Miller, International Finance Corporation
Stéphane Dees, Banque de France and Bordeaux School of Economics, University of Bordeaux, France,Selin Ozyurt-Miller, International Finance Corporation
Financial stability is essential for sustainable economic growth, and prudential policies have been reinforced since the Global Financial Crisis (GFC) to safeguard this stability. The Basel III framework introduced stringent capital, liquidity, and risk management requirements for banks, strengthening their resilience. In the face of growing climate-related risks, central banks and supervisory authorities must ensure that financial systems remain stable. Extreme weather events and abrupt transitions to a low-carbon economy can lead to significant financial losses, including asset stranding and increased defaults, threatening overall financial stability. Central banks and supervisory authorities must integrate climate risks into their financial supervision frameworks, adapting existing tools to manage these complex, systemic risks. Prudential responses must encompass both individual institutions and broader financial systems to mitigate the impact of climate change on financial stability. Ensuring a resilient financial system is crucial for maintaining economic stability in the transition to a low-carbon future.
The chapter describes the basic terminology used in the book, the composition of the Earth system and the principles of climate dynamics. It details the main components of the Earth system (atmosphere, ocean, hydrosphere, cryosphere, biosphere and solid Earth) and processes relevant to understanding climate dynamics. The concepts of climate, climate variability and climate change are discussed in the context of Quaternary climate dynamics. The global cycles of energy, water and carbon and their importance for climate evolution and variability are presented. The chapter introduces the mechanisms behind different types of radiative forcing, climate feedbacks and climate sensitivity. The difference between equilibrium and transient climate responses to different climate forcings is specified. The frameworks of stability and instability are introduced and discussed in application to climate. The relationship between the stochasticity of the Earth system and the predictability of climate change is presented.
The effects of confinement and polydispersity on the shear-induced diffusivity of non-Brownian, neutrally buoyant spheres suspended in a Newtonian fluid are investigated using simulations that incorporate short-range lubrication forces, surface roughness and frictional contacts. Simulations were performed at a fixed volume fraction of 0.45 for multiple values of particle roughness and friction coefficient. Confinement by bounding walls promoted layered structures that suppressed particle mobility and reduced diffusivity, while also diminishing the influence of friction and roughness. In contrast, high polydispersity disrupted layering and enhanced diffusivity, even in confined systems. Polydispersity also led to size-dependent demixing, with smaller particles preferentially migrating towards the walls and exhibiting higher mobility. These results have implications for modelling and controlling transport in suspensions, where confinement and polydispersity alter the effects of friction and roughness on shear-induced diffusion.
The chapter outlines the primary methods used in empirical paleoclimatology, beginning with an overview of key paleoclimate proxies (stable oxygen and carbon isotopes, atmospheric composition, ice-rafted debris, aeolian dust and pollen) and the past environmental conditions they help reconstruct. The applicability and potential limitations of different proxies are discussed. It then describes the main paleoclimate archives, such as marine sediments and ice cores, speleothems, tree rings and others, in relation to paleoclimate proxies. The main dating techniques used in Quaternary paleoclimatology, such as the radiocarbon method, paleomagnetism and orbital tuning, are briefly examined. Several important paleoclimatological stacked records are presented, such as the Lisiecki-Raymo benthic stack. Finally, the main applications of paleoclimate proxies for reconstructing paleoenvironments and understanding past climate change and data-model comparison are reviewed.
The Quaternary period, which began 2.58 million years ago and continues to the present day, is distinctive for its significant climate variability. Understanding the mechanisms of climate change during this period and the relationship between carbon dioxide levels and temperature is hugely important in improving our ability to develop models to predict future climate change. This book discusses the main methods of empirical climatology and the models used to address different aspects of Quaternary climate dynamics, offering a multidisciplinary view of past and future climate changes. It examines the proposed mechanisms of Quaternary climate variability, including glacial cycles and abrupt climate changes, and their relationship to the intrinsic instability of ocean circulation and ice sheets. Including a final chapter on the Anthropocene, it provides a comprehensive overview of Quaternary and modern climate dynamics for graduate students and researchers working in paleoclimatology and climate change science.
The classical problem of steady rarefied gas flow past an infinitely thin circular disk is revisited, with particular emphasis on the gas behaviour near the disk edge. The uniform flow is assumed to be perpendicular to the disk surface. An integral equation for the velocity distribution function, derived from the linearised Bhatnagar–Gross–Krook model of the Boltzmann equation and subject to diffuse reflection boundary conditions, is solved numerically. The numerical method fully accounts for the discontinuity in the velocity distribution function that arises due to the presence of the edge. It is found that a kinetic boundary layer forms near the disk edge, extending over several mean free paths, and that its magnitude scales as $\textit{Kn}^{1/2}$ as the Knudsen number $\textit{Kn}$ (defined with respect to the disk radius) tends to zero. A thermal polarisation effect, previously studied for spherical geometries, is also observed in the disk case, with a more pronounced manifestation near the edge that exhibits the same $\textit{Kn}^{1/2}$ scaling. The drag force acting on the disk is computed over a wide range of Knudsen numbers and shows good agreement with existing results for a hard-sphere gas and in the near-free-molecular regime.
In Navier–Stokes (NS) turbulence, large-scale turbulent flows inevitably determine small-scale flows. Previous studies using data assimilation with the three-dimensional (3-D) NS equations indicate that employing observational data resolved down to a specific length scale, $\ell ^{\rm 3\text{-}D}_{\ast }$, enables the successful reconstruction of small-scale flows. Such a length scale of ‘essential resolution of observation’ for reconstruction $\ell ^{\rm 3\text{-}D}_{\ast }$ is close to the dissipation scale in three-dimensional NS turbulence. Here, we study the equivalent length scale in two-dimensional (2-D) NS turbulence, $\ell ^{\rm 2\text{-}D}_{\ast }$, and compare with the three-dimensional case. Our numerical studies using data assimilation and conditional Lyapunov exponents reveal that, for Kolmogorov flows with Ekman drag, the length scale $\ell ^{\rm 2\text{-}D}_{\ast }$ is actually close to the forcing scale, substantially larger than the dissipation scale. Furthermore, we discuss the origin of the significant relative difference between the length scales, $\ell ^{\rm 2\text{-}D}_{\ast }$ and $\ell ^{\rm 3\text{-}D}_{\ast }$, based on inter-scale interactions, ‘cascades’ and orbital instabilities in turbulence dynamics.
Stéphane Dees, Banque de France and Bordeaux School of Economics, University of Bordeaux, France,Selin Ozyurt-Miller, International Finance Corporation
Scientists have long warned about the severe environmental consequences if global temperatures continue to rise. According to the 2021 IPCC report, the Earth's temperature has increased by 1.1°C above preindustrial levels, and the world is projected to exceed 1.5°C within two decades, even with emission reduction efforts. International initiatives, starting with the 1992 UNFCCC and the 1997 Kyoto Protocol, laid the groundwork for climate action. The 2015 Paris Agreement, a pivotal moment, set a goal to limit warming to below 2°C, ideally 1.5°C, through nationally determined contributions (NDCs). Addressing climate change requires systemic shifts in economic structures, moving away from fossil fuels toward renewable energy, promoting decarbonization, and emphasizing resource efficiency. While transitioning to a low-carbon economy poses initial costs, the long-term benefits include reduced environmental damage, better health, and enhanced energy efficiency. The ongoing global cooperation and economic transformation are crucial for mitigating climate change impacts.
After sunlight, wind has the most practical potential to supply the world’s all-purpose energy demand. Not only are wind resources abundant in almost every country, but the cost of onshore wind energy has also declined so much that, in 2024, onshore wind, along with utility PV, was the least expensive form of new electricity in many countries. Its low cost has resulted in massive wind installations to replace fossil-fuel power plants and to supply new energy demand. This chapter discusses the history of windmills and wind turbines, followed by a discussion of the different types of wind turbines and wind-turbine components. The chapter also discusses how wind turbines work and how generators convert the mechanical energy from a rotating blade into electricity. Finally, the chapter discusses the wind-farm footprint and spacing areas needed to power the world, wind resources available worldwide, and the impacts of wind turbines on global wind speeds, global temperatures, hurricanes, birds, and bats.